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Table 9

Space velocities for members and candidate members of the Chamaeleon associations.

Name U V W U LSR V LSR W LSR Notes
(km s-1) (km s-1) (km s-1) (km s-1) (km s-1) (km s-1)

Chamaeleon I cloud
T3A −1.8 ± 7.3 −13.2 ± 3.4 −4.6 ± 5.8 −10.3 0.2 1.9
SY Cha 8.5 ± 3.3 −17.5 ± 1.4 −4.8 ± 2.5 −0.0 −4.1 1.7
Sz 4 −1.1 ± 5.3 −16.3 ± 3.2 −7.4 ± 5.6 −9.6 −2.9 −0.9
TW Cha 5.9 ± 1.7 −19.0 ± 1.3 −7.0 ± 1.6 −2.6 −5.7 −0.5
CR Cha 7.6 ± 1.5 −18.8 ± 1.0 −7.3 ± 1.6 −0.9 −5.5 −0.8
CS Cha 7.9 ± 1.5 −19.1 ± 1.0 −6.6 ± 2.1 −0.6 −5.7 −0.1
CT Cha 6.1 ± 1.6 −18.0 ± 0.8 −8.6 ± 1.3 −2.4 −4.6 −2.2
T21 14.3 ± 3.3 −20.9 ± 1.4 −8.8 ± 2.0 5.8 −7.5 −2.3
DI Cha 3.4 ± 1.5 −13.8 ± 1.0 −11.8 ± 1.3 −5.1 −0.4 −5.3
VV Cha 6.0 ± 1.9 −17.6 ± 1.4 −11.2 ± 1.5 −2.5 −4.2 −4.7
VW Cha 6.1 ± 1.6 −17.5 ± 1.2 −10.5 ± 2.4 −2.4 −4.1 −4.9
CHXR 37 8.7 ± 2.8 −16.6 ± 3.4 −10.4 ± 6.7 0.2 −3.2 −3.9
VZ Cha 6.1 ± 1.7 −17.5 ± 1.2 −10.5 ± 2.4 −2.4 −4.1 −4.0
T46 8.8 ± 1.9 −16.5 ± 1.2 −10.0 ± 1.5 0.3 −3.1 −3.6
CHXR 47 7.4 ± 1.9 −17.5 ± 1.9 −8.5 ± 1.6 −1.1 −4.2 −2.0
CHX 18N 8.5 ± 3.3 −17.5 ± 1.4 −4.8 ± 2.5 −0.0 −4.1 1.7
CHX 20 14.3 ± 3.3 −20.9 ± 1.4 −8.8 ± 2.0 5.8 −7.5 −2.3
CV Cha 6.1 ± 5.0 −18.3 ± 1.8 −8.1 ± 2.9 −2.4 −4.9 −1.6 (1)
RX J1129.2-7546 10.8 ± 2.0 −16.2 ± 2.0 −10.0 ± 1.3 2.3 −2.8 −3.5
RX J1158.5-7913 5.7 ± 2.8 −16.1 ± 2.3 −8.8 ± 1.7 −2.8 −2.8 −2.3 (2)
Mean values (σ) 7.0 (3.8) −17.4 (1.9) −8.4 (2.1) −1.5 (3.8) −4.1 (1.9) −2.0 (2.1)

Chamaeleon II cloud
Sz 46N 2.0 ± 5.5 −25.0 ± 2.9 15.4 ± 15.9 −6.5 −11.6 21.9
IRAS 12535-7623 14.7 ± 3.3 −18.4 ± 2.4 −12.0 ± 2.4 6.2 −5.1 −5.6
Sz 50 12.4 ± 3.5 −21.9 ± 2.5 −7.7 ± 3.1 3.9 −8.5 −1.2
RX J1303.1-7706 16.6 ± 2.7 −24.0 ± 1.8 −7.8 ± 1.5 8.1 −10.6 −1.3
Hn 23 −14.5 ± 16.8 −12.6 ± 11.4 11.5 ± 18.1 −23.0 0.8 18.0
Sz 58 14.0 ± 6.9 −22.1 ± 5.7 −8.2 ± 3.8 5.5 −8.7 −1.7
Sz 59 8.5 ± 2.7 −17.5 ± 2.6 −12.7 ± 3.0 0.0 −4.2 −6
Sz 60W 30.5 ± 14.4 −34.8 ± 10.1 −6.6 ± 4.8 22.0 −21.4 −0.1
Sz 61 12.0 ± 2.9 −20.7 ± 2.9 −6.9 ± 1.8 3.5 −7.4 −0.4
Mean values (σ) 10.7 (11.4) −21.9 (5.8) −3.9 (9.5) 2.2 (11.4) −8.5 (5.8) 2.6 (9.5)

ϵ Chamaeleontis cluster
CM Cha 9.6 ± 4.8 −26.3 ± 3.3 1.0 ± 4.8 1.1 −13.0 7.5 (3)
T Cha 18.1 ± 13.6 −28.9 ± 7.5 −16.9 ± 3.6 9.6 −15.5 −10.4 (1, 4)
DW Cha 12.2 ± 1.5 −19.9 ± 1.9 −9.1 ± 0.7 3.7 −6.5 −2.6
RX J1159.7-7601 12.3 ± 1.6 −19.7 ± 1.9 −10.3 ± 1.0 3.8 −6.3 −3.9
HD 104467 14.0 ± 1.4 −17.1 ± 1.8 −9.5 ± 0.6 5.5 −3.7 −3.0
RX J1219.7-7403 12.7 ± 2.3 −21.1 ± 2.1 −8.5 ± 1.1 4.2 −7.7 −2.0
RX J1239.4-7502 11.9 ± 1.8 −20.6 ± 1.9 −10.8 ± 1.3 3.4 −7.2 −4.3
DZ Cha 13.8 ± 1.9 −18.3 ± 1.9 −12.8 ± 1.1 5.3 −4.9 −6.3
GSC 9420-0948 16.3 ± 2.0 −13.1 ± 2.0 −7.5 ± 1.1 7.8 0.3 −1.0
GSC 9416-1029 12.7 ± 1.4 −17.6 ± 1.8 −7.5 ± 1.2 4.2 −4.2 −1.0
GSC 9239-1572 9.4 ± 1.8 −24.9 ± 1.9 −8.9 ± 1.0 0.9 −11.5 −2.4
CP-68 1388 11.3 ± 1.3 −21.2 ± 0.6 −6.8 ± 1.2 2.8 −7.8 −0.3
HD 105923 10.1 ± 1.4 −20.6 ± 0.8 −9.8 ± 0.9 1.6 −7.2 −3.3
GSC 9415-2676 11.2 ± 1.8 −18.5 ± 1.9 −11.3 ± 1.2 2.7 −5.1 −4.8
CD-69 1055 11.7 ± 1.4 −21.7 ± 0.9 −10.0 ± 0.7 3.2 −8.3 −3.5
MP Mus 12.0 ± 0.9 −21.6 ± 0.6 −9.3 ± 0.9 3.5 −8.2 −2.8
RX J1123.2-7924 7.3 ± 1.5 −9.9 ± 1.9 −17.2 ± 1.0 −1.2 3.5 −10.7 (5)
RX J1216.8-7753 10.2 ± 1.5 −19.8 ± 1.8 −10.3 ± 0.8 1.7 −6.4 −3.8
Mean values (σ) 12.1 (2.4) −20.0 (4.1) −9.7 (3.7) 3.6 (2.4) −6.6 (4.1) −3.2 (3.7)

η Chamaeleontis cluster
EG Cha 9.5 ± 0.9 −20.0 ± 1.4 −11.1 ± 1.6 1.0 −6.7 −4.6
EM Cha 15.0 ± 1.2 −8.4 ± 1.7 −6.6 ± 1.8 6.5 4.9 −0.1
EO Cha 11.8 ± 1.2 −17.6 ± 1.5 −11.0 ± 1.7 3.3 −4.2 −4.6
EQ Cha 11.4 ± 1.1 −20.7 ± 1.5 −11.7 ± 1.7 2.9 −7.3 −5.2
RX J0850.1-7554 10.3 ± 0.8 −20.2 ± 1.4 −2.7 ± 1.6 1.8 −6.9 3.8
RX J0902.9-7759 13.4 ± 1.1 −14.2 ± 1.5 −9.9 ± 1.6 4.9 −0.8 −3.4
RX J0915.5-7608 7.7 ± 1.2 −22.8 ± 1.5 −11.0 ± 1.5 −0.8 −9.4 −4.5
HD 82879 7.0 ± 1.0 −19.2 ± 1.5 −8.3 ± 1.4 −1.5 −5.8 −1.8
RX J0935.0-7804 9.4 ± 1.0 −17.4 ± 1.6 −7.5 ± 1.4 0.9 −4.0 −1.1
HD 86356 13.4 ± 0.9 −20.7 ± 1.6 0.9 ± 1.4 4.9 −7.3 7.4
RX J1001.1-7913 12.5 ± 1.1 −20.9 ± 1.8 2.0 ± 1.6 4.0 −7.6 8.6
RX J1140.3-8321 12.7 ± 1.2 −21.7 ± 1.8 2.5 ± 1.2 4.2 −8.3 8.9
Mean values (σ) 11.2 (2.3) −18.7 (3.8) −6.2 (5.2) 2.7 (2.3) −5.3 (3.8) 0.3 (5.2)

Notes.(1) The distance inferred from the Hipparcos parallax (Table 5) was used in the calculation. (2) Assuming the distance to ϵ Cha for this star, the following space velocities are obtained (U,V,W) = (2.0 ± 2.0, −14.5 ± 2.0, −7.2 ± 1.2) km s-1. (3) If the distance to Cha II is assumed for this object, the resulting space velocities are (U,V,W) = (20.6 ± 8.0, −34.5 ± 5.5,3.9 ± 7.7) km s-1. (4) With a parallax π = 15.06 ± 3.31, we obtain for this star (U,V,W) = (1.5 ± 7.0, −21.5 ± 8.1, −10.2 ± 3.7) km s-1. (5) Assuming the distance to Cha II for this star, we obtain (U,V,W) = (14.5 ± 3.2, −10.8 ± 2.4, −25.7 ± 1.6) km s-1.

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